Multifrequency study of a double–double radio galaxy J0028+0035

A. Marecki, M. Jamrozy, J. Machalski, U. Pajdosz-Śmierciak
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引用次数: 3

Abstract

We report discovery of a double-double radio source (DDRS) J0028+0035. We observed it with LOFAR, GMRT, and the VLA. By combining our observational data with those from the literature, we gathered an appreciable set of radio flux density measurements covering the range from 74 MHz to 14 GHz. This enabled us to carry out an extensive review of physical properties of the source and its dynamical evolution analysis. In particular, we found that, while the age of the large-scale outer lobes is about 245 Myr, the renewal of the jet activity, which is directly responsible for the double-double structure, took place only about 3.6 Myr ago after about 11 Myr long period of quiescence. Another important property typical for DDRSs and also present here is that the injection spectral indices for the inner and the outer pair of lobes are similar. The jet powers in J0028+0035 are similar too. Both these circumstances support our inference that it is in fact a DDRS which was not recognized as such so far because of the presence of a coincident compact object close to the inner double so that the centre of J0028+0035 is apparently a triple.
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双双射电星系J0028+0035的多频研究
我们报告发现了一个双双射电源(DDRS) J0028+0035。我们用LOFAR, GMRT和VLA观察了它。通过将我们的观测数据与文献中的数据相结合,我们收集了一组可观的无线电通量密度测量值,范围从74兆赫到14千兆赫。这使我们能够对源的物理性质进行广泛的审查,并对其动态演变进行分析。特别是,我们发现,虽然大尺度外叶的年龄约为245 Myr,但直接导致双双结构的射流活动的更新仅发生在大约11 Myr的长时间静止后的3.6 Myr左右。ddrs的另一个重要特征是,内部和外部叶对的注入光谱指数是相似的。J0028+0035的飞机动力也很相似。这两种情况都支持了我们的推断,即它实际上是一个DDRS,到目前为止还没有被识别出来,因为在靠近内部双星的地方有一个重合的致密天体,所以J0028+0035的中心显然是一个三星。
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